Add to ORKGResearch was carried out on developing a flow field interaction model for both the dayside and nightside ionosphere of Venus. Specific topics related to the dayside ionosphere included: (1) wave particle mechanisms at the ionopause, (2) structure and dynamics of the Venus ionopause and Ionosphere, and (3) flows and fields in the Venus Ionosphere. The structure and dynamics of ion troughs was also studied in the nightside ionosphere of Venus
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
Our understanding of the physical and chemical processes which control the behavior of the Venus ion...
Model calculations of the dayside ionosphere of Venus are presented. The coupled continuity and mome...
A combination of numerical modeling and analysis of the Pioneer Venus UADS data base is studied, spe...
The upper atmosphere and ionosphere of Venus have been explored by a series of Mariner and Venera sp...
The current state of knowledge of the chemistry, dynamics and energetics of the upper atmosphere and...
The aeronomy experiments on the Pioneer Venus Orbiter (PVO) have established three characteristic fe...
A population of low-energy (0-250 V E/q) ions with tailward directed velocity vectors and energies a...
Venus is a slowly rotating planet with a measured night-time ionosphere. The mechanism by which the ...
AbstractThe transterminator ion flow in the Venusian ionosphere is observed at solar minimum for the...
Magnetometer measurements on the Pioneer Venus Orbiter (PVO) have shown that Venus is a non-magnetic...
Topside ionosphere of Venus and interaction with solar wind using Mariner 5 two frequency experimen
An attempt is made to establish an ionization source capable of maintaining the nighttime Venus iono...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
Our understanding of the physical and chemical processes which control the behavior of the Venus ion...
Model calculations of the dayside ionosphere of Venus are presented. The coupled continuity and mome...
A combination of numerical modeling and analysis of the Pioneer Venus UADS data base is studied, spe...
The upper atmosphere and ionosphere of Venus have been explored by a series of Mariner and Venera sp...
The current state of knowledge of the chemistry, dynamics and energetics of the upper atmosphere and...
The aeronomy experiments on the Pioneer Venus Orbiter (PVO) have established three characteristic fe...
A population of low-energy (0-250 V E/q) ions with tailward directed velocity vectors and energies a...
Venus is a slowly rotating planet with a measured night-time ionosphere. The mechanism by which the ...
AbstractThe transterminator ion flow in the Venusian ionosphere is observed at solar minimum for the...
Magnetometer measurements on the Pioneer Venus Orbiter (PVO) have shown that Venus is a non-magnetic...
Topside ionosphere of Venus and interaction with solar wind using Mariner 5 two frequency experimen
An attempt is made to establish an ionization source capable of maintaining the nighttime Venus iono...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...
The major mechanisms for maintenance of the nightside ionosphere of Venus have been the subject of m...